射频天线螺旋度与螺旋子源中的粒子加热有关

K J Stevenson, T J Gilbert, T N Good, M Paul, P Shi, R Nirwan, P Srivastav, T E Steinberger, E E Scime
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摘要

实验证明,离子现象(如低混合共振)在螺旋光源的运行中发挥着重要作用。在氦光子源边缘的有界啸波慢分支(即 Trivelpiece-Gould 模式)的阻尼与高能电子的产生、等离子体边缘的离子加热和各向异性离子加热有关。在这里,我们展示了离子速度分布函数测量结果、电子密度和温度测量结果,以及在螺旋子源中 m=|1| 螺旋天线两侧的磁波动测量结果,它们是驱动频率、磁场强度和磁场方向相对于天线螺旋度的函数。在与 m=+1 模式发射一致的天线一侧,出现了显著的电子和离子加热现象(高达两倍)。电子和离子加热发生在等离子体边缘的一个电子皮层深度内,这里预计会出现慢波阻尼。粒子加热增强的源参数也与较低的混合共振效应相一致,而混合共振效应只有在 Trivelpiece-Gould 波激发时才会出现。
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RF antenna helicity dependent particle heating in a helicon source
Experiments have demonstrated that ion phenomena, such as the lower hybrid resonance, play an important role in helicon source operation. Damping of the slow branch of the bounded whistler wave at the edge of a helicon source (i.e. the Trivelpiece-Gould mode) has been correlated with the creation of energetic electrons, heating of ions at the plasma edge, and anisotropic ion heating. Here we present ion velocity distribution function measurements, electron density and temperature measurements, and magnetic fluctuation measurements on both sides of an m=|1| helical antenna in a helicon source as a function of the driving frequency, magnetic field strength, and magnetic field orientation relative to the antenna helicity. Significant electron and ion heating (up to two times larger) occurs on the side of the antenna consistent with the launch of the m=+1 mode. The electron and ion heating occurs within one electron skin depth of the plasma edge, where slow wave damping is expected. The source parameters for enhanced particle heating are also consistent with lower hybrid resonance effects, which can only occur for Trivelpiece-Gould wave excitation.
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